Mantle convection is the process by which heat from the Earth's interior causes the movement of the semi-fluid mantle layer, which lies between the Earth's crust and the outer core. This process is a key mechanism in plate tectonics, influencing the movement of tectonic plates on the Earth's surface. Here’s how mantle convection works: 1. **Heat Production**: The Earth's interior generates heat through radioactive decay and residual heat from the planet’s formation.
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Mantle convection is buoyancy-driven motion in a rocky planetary mantle. Heating and cooling create density differences; chemical and mineral-phase differences can also affect buoyancy. Although the mantle is mostly solid, deformation by material creep permits slow flow over geological time.
A simple model balances viscous resistance with buoyancy and transports heat by both flow and thermal conduction. Its Rayleigh number compares those effects. Temperature-dependent mantle viscosity and the strength of the lithosphere help determine whether the surface moves as plates or remains a stagnant lid. Seismic structure, surface deformation and heat flux constrain different parts of this model.